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<ri:Resource created="2022-01-13T12:35:45Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>New M87 GCs metallicities from Keck &amp; MMT sp.</title><shortName>J/ApJ/900/95</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/95</identifier><altIdentifier>doi:10.26093/cds/vizier.19000095</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Villaume A.</name></creator><creator><name>Foreman-Mackey D.</name></creator><creator><name>Romanowsky A.J.</name></creator><creator><name>Brodie J.</name></creator><creator><name>Strader J.</name></creator><date role="Updated">2022-10-04T12:00:15Z</date><date role="Created">2022-01-13T12:35:45Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>metallicity</subject><subject>globular-star-clusters</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present an extensive study of spectroscopically derived chemical abundances for M87 and its globular cluster (GC) system. Using observations from the Mitchell spectrograph at McDonald, LRIS at Keck, and Hectospec on the MMT, we derive new metallicity gradients from ~2 to 140kpc. We use a novel hierarchical statistical framework to simultaneously separate the GC system into subpopulations while measuring the metallicity gradients of those subpopulations. We create physically motivated spectral stacks of the GC subpopulations by leveraging the output of this statistical framework to perform the first application of abundance tagging in a massive early-type galaxy to better constrain the origins of the GC subpopulations and thus the assembly history of M87. We find a metal-poor, {alpha}-enhanced population of GCs in both the inner and outer halos unanticipated by current cosmological simulations of galaxy evolution. We use the remarkably flat metallicity gradients we find for both the metal-rich and metal-poor GC subpopulations in the inner halo as tentative evidence that some amount of the metal-poor GCs formed directly in the halo of M87 at high redshift.</description><source format="bibcode">2020ApJ...900...95V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/95</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/1841">J/AJ/120/1841 : Abund. &amp; Kinematics of Halo and Disk Stars (Fulbright 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/414/503">J/A+A/414/503 : Abundances in the Sgr dSph (Bonifacio+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/1117">J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. 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